Relaxing the Higgs Mass and Its Vacuum Energy by Living at the Top of the Potential

PHYSICAL REVIEW D 101, 115002 (2020) Relaxing the Higgs mass and its vacuum energy by living at the top of the potential † Alessandro Strumia1,* and Daniele Teresi 1,2, 1Dipartimento di Fisica “E. Fermi”, Universit`a di Pisa, Largo Bruno Pontecorvo 3, I-56127 Pisa, Italy 2INFN, Sezione di Pisa, Largo Bruno Pontecorvo 3, I-56127 Pisa, Italy (Received 17 February 2020; accepted 19 May 2020; published 1 June 2020) We consider an ultralight scalar coupled to the Higgs in the presence of heavier new physics. In the electroweak broken phase the Higgs gives a tree-level contribution to the light-scalar potential, while new physics contributes at loop level. Thereby, the theory has a cosmologically metastable phase where the light scalar is around the top of its potential, and the Higgs is a loop factor lighter than new physics. Such regions with precarious naturalness are anthropically and environmentally selected, as regions with heavier Higgs crunch quickly. We expect observable effects of rolling in the dark-energy equation of state. Furthermore, vacuum energies up to the weak scale can be canceled down to anthropically small values. DOI: 10.1103/PhysRevD.101.115002 I. INTRODUCTION values of ϕ such that the Higgs mass is a loop factor lighter than new physics. Scalars with mass m below the present Hubble scale H0 This observation is relevant for the Higgs-mass hierarchy can still lie away from the minimum of their potential and problem if, for some reason, ϕ lies close to the maximum of thereby undergo significant cosmological evolution at its potential. The authors of [7,8] explored possible reasons: present times. This can be of possible relevance for barring the possibility that ϕ is a ghost, they added extra understanding the apparently unnatural hierarchy of scales wiggles to Vϕ in order to generate local minima around the observed in Nature: cosmological constant much below the maximum, arguing that they can be favored cosmologically weak scale much below the Planck scale. See [1–12] for because they inflate more. some recent attempts of understanding hierarchies via We consider a simpler way of living at the top. Since the cosmological evolution. potential Vϕ is flat around its maximum, regions suffi- We here consider a scalar ϕ with the shift symmetry that ciently close to it can be cosmologically metastable, as long keeps its potential flat broken by small interactions to other as ϕ is so weakly coupled that its mass is small, m ≲ H0. fields, in particular to the Higgs doublet H and to other Instead, regions away from the maximum quickly roll heavier new physics that generates a Higgs mass hierarchy down and catastrophically collapse into a big crunch, as problem. The interaction with the Higgs can be para- illustrated in Fig. 1. In this way, only regions where the ϕ M2ðϕÞ metrized by a -dependent Higgs mass, h . The model Higgs is light are long-lived: a small Higgs mass is selected. will cosmologically generate a little hierarchy, maximal in ϕ The multiverse volume at late times gets dominated by such the special case where the couplings to new physics are near-critical regions at the border between the broken and mediated by the Higgs. unbroken Higgs phase. Indeed, integrating out the Higgs generates a tree-level We also find that this setting allows for a range of values ∼− 4ðϕÞ negative contribution Vϕ Mh to the effective poten- of the vacuum energy, up to the weak scale in the most ϕ 2ðϕÞ 0 tial for if Mh > , i.e., when electroweak symmetry optimistic case, thereby providing a mechanism (alternative breaking takes place. Heavier new physics contributes at to a landscape of vacua) for the anthropic selection of loop level. The full potential Vϕ can have a maximum for the cosmological constant down to the small observed value. *[email protected] This scenario generates a little hierarchy, making the † [email protected] weak scale one or two loop factors below the scale of new physics. The needed new physics is unspecified and might Published by the American Physical Society under the terms of be a full solution to hierarchy problems, such as super- the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to symmetry (see, e.g., [8]), or possibly a landscape with the author(s) and the published article’s title, journal citation, electroweak, rather than meV, spacing (e.g., from string and DOI. Funded by SCOAP3. [13–15] or quantum field [16,17] theory). 2470-0010=2020=101(11)=115002(8) 115002-1 Published by the American Physical Society ALESSANDRO STRUMIA and DANIELE TERESI PHYS. REV. D 101, 115002 (2020) couplings g.2 For example, the heavy new physics could be supersymmetric and ϕ could be a quasimodulus. We want to compute the effective potential for ϕ. First, we integrate out the heavy new physics obtaining the effective field theory around the weak scale, with effective potential 2ðϕÞ ð ϕÞ¼ − Mh j j2 þ λj j4 þ heavyðϕÞ ð Þ Veff H; V0 2 H H Vϕ ; 1 where λ ≈ 0.126 is the Higgs quartic. The potential contains the tree-level coupling of ϕ to the Higgs, parametrized by 2ðϕÞ FIG. 1. Effective potential for ϕ around its maximum. After Mh . The squared Higgs mass might receive unnaturally inflation different patches of the Universe have different values of large corrections from heavy new physics, but what matters ϕ. In most patches ϕ is away from its maximum and slides down here is its value renormalized around the weak scale. In leading to a crunch. Only patches where ϕ is near the top are agreement with the decoupling theorem, heavy new physics metastable on cosmological timescales. These correspond to a heavy can instead give the Vϕ ðϕÞ term in the effective potential Higgs mass one or two loop factors lighter than new physics. (to be computed at one- or two-loop level in Sec. II A). 2ðϕÞ 0 Finally, we integrate out the Higgs boson. If Mh > An observable consequence of precarious naturalness is (such that, in our notation, the electroweak symmetry is that in an Oð1Þ fraction of the long-lived regions of the broken), the Higgs gives a tree-level contribution to ðϕÞ Universe, the scalar field ϕ is rolling down the potential Veff . The Higgs also gives a loop-level contribution, now, with detectably large effects on the equation of state of the usual running of the cosmological constant, that can be dark energy. The other robust consequence is the presence neglected with respect to loop effects of heavier fields. We of new physics coupled to the Higgs around or below the thereby obtain the effective potential for the light field ϕ ≈20 TeV scale, in order to generate the maximum at the observed value. 4ðϕÞ Mh 2 heavy V ðϕÞ¼ 0 − θð ðϕÞÞ þ ðϕÞ ð Þ The paper is structured as follows. In Sec. II we present eff V 16λ Mh Vϕ ; 2 the model and study its cosmological dynamics in Sec. III, where we illustrate the mechanism leading to precarious θ ¼ 1 M2ðϕÞ > 0 naturalness. We then discuss bounds and signals in Sec. IV where for h and zero otherwise, so that the ðϕÞ ϕ 0 tree-level part of Veff is flat for < . and finally conclude in Sec. V. heavy We assume that the sign of Vϕ is such that, together ðϕÞ with the negative tree-level Higgs term, Veff has a local II. PRECARIOUS NATURALNESS: THE SETUP maximum. Without loss of generality, we can shift ϕ so that ϕ ¼ 0 We consider the Standard Model (SM) with mass the maximum lies at . We next assume, for simplicity, scale M ≈ 125 GeV plus heavier new physics at the mass that the two terms can be approximated by first-order h Taylor expansions scale M ≫ Mh and an ultralight scalar ϕ with mass-scale m ≪ Mh. A Higgs-mass hierarchy problem arises if the Higgs 2ðϕÞ ≃ 2 þ ϕ heavy ≃ ϕ ð Þ Mh Mh0 g ;Vϕ gA : 3 interacts significantly with heavier new particles. We leave the heavy new physics unspecified. This includes the possibility of new physics, such as supersymmetry, that The parameter Mh0 must be negligibly different from the ϕ makes its scale M naturally smaller than the ultimate physical Higgs mass, 125 GeV, given that will lie very Λ close to the maximum. The maximum condition then cutoff of the theory at some scale , possibly around 2 1 ¼ 8λ the Planck mass. implies Mh0 A. As we now show, this is loop sup- On the other hand, the lightness of ϕ is naturally pressed with respect to M. understood if the ϕ potential is protected by a shift symmetry, broken at some scale ≲Λ by very small 2Such tiny couplings mediate a force much weaker than gravity for the Higgs. However, this is not in contradiction with the weak gravity conjecture [18], since the force is attractive, so that its effect adds up to gravity [19]. Sometimes it is argued that 1The possibility of new physics at the weak scale that makes also scalar forces must be stronger than gravity [19], but the the Higgs mass natural would have been simpler, but it has been arguments for this are weaker [20] and disappear for fields with disfavored by collider searches. sizable gauge interactions, like the Higgs boson in our case. 115002-2 RELAXING THE HIGGS MASS AND ITS VACUUM … PHYS. REV. D 101, 115002 (2020) FIG. 2. Combined selection of a small cosmological constant, in addition to a small Higgs mass, for m ≪ H0.

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